<?xml version="1.0" encoding="UTF-8"?>
<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Dark matter from scalar field fluctuations · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/1905.01214/</link><description>Collected HN comments and submissions linking this paper.</description><language>en</language><lastBuildDate>Mon, 02 Nov 2026 11:16:22 GMT</lastBuildDate><atom:link href="https://hackerpaper.kaipfister.de/p/1905.01214/feed.xml" rel="self" type="application/rss+xml" /><item><title>Dark matter from scalar field fluctuations — mentioned by raattgift</title><link>https://news.ycombinator.com/item?id=20663475</link><guid isPermaLink="false">urn:hackerpapers:mention:1905.01214:20663475</guid><pubDate>Sat, 10 Aug 2019 17:46:24 GMT</pubDate><description>&lt;p&gt;The paper proposes that the entirety of dark matter is a massive free (as in non-interacting and non-self-interacting) field that appeared at the end of inflation, but before big bang nucleosynthesis (&amp;quot;BBN&amp;quot;). In order to make this work with observations of the cosmic microwave background, the field has to have much lower mass earlier during inflation than at inflation&amp;#x27;s end. The mass-gaining mechanism is not elucidated. There is only one known scalar field -- the Higgs -- and it is far from a free field. Any non-gravitational interaction between this proposed field and the rest of the…&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1905.01214/"&gt;Paper and discussion history&lt;/a&gt;. A mention is not an endorsement.&lt;/p&gt;</description><category>astro-ph.CO</category></item><item><title>Dark matter from scalar field fluctuations — mentioned by raattgift</title><link>https://news.ycombinator.com/item?id=20663162</link><guid isPermaLink="false">urn:hackerpapers:mention:1905.01214:20663162</guid><pubDate>Sat, 10 Aug 2019 16:57:23 GMT</pubDate><description>&lt;p&gt;&amp;gt; Can anyone explain I&amp;#x27;ll try. The tl;dr is at the end before my own footnote. The author certainly doesn&amp;#x27;t make it easy, even for people familiar with the standard model of cosmology. The very first sentence of the paper [ https://arxiv.org/abs/1905.01214 ] reads, &amp;quot;Dark matter (DM) may have its origin in a pre-big-bang epoch. It may have been produced, for example, by decays or annihilations of particles during the Big Bang, i.e. by the so-called ’freeze-in’ [1–3] mechanism, or by e.g. the misalignment mechanism which generated a non-zero DM abundance during cosmic inflation (see e.g.…&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1905.01214/"&gt;Paper and discussion history&lt;/a&gt;. A mention is not an endorsement.&lt;/p&gt;</description><category>astro-ph.CO</category></item><item><title>Dark matter from scalar field fluctuations — mentioned by saagarjha</title><link>https://news.ycombinator.com/item?id=20655412</link><guid isPermaLink="false">urn:hackerpapers:mention:1905.01214:20655412</guid><pubDate>Fri, 09 Aug 2019 15:46:04 GMT</pubDate><description>&lt;p&gt;PDF on arXiv: https://arxiv.org/pdf/1905.01214.pdf&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1905.01214/"&gt;Paper and discussion history&lt;/a&gt;. A mention is not an endorsement.&lt;/p&gt;</description><category>astro-ph.CO</category></item><item><title>Dark matter from scalar field fluctuations — mentioned by ISL</title><link>https://news.ycombinator.com/item?id=20655029</link><guid isPermaLink="false">urn:hackerpapers:mention:1905.01214:20655029</guid><pubDate>Fri, 09 Aug 2019 15:06:21 GMT</pubDate><description>&lt;p&gt;ArXiv link: https://arxiv.org/abs/1905.01214&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1905.01214/"&gt;Paper and discussion history&lt;/a&gt;. A mention is not an endorsement.&lt;/p&gt;</description><category>astro-ph.CO</category></item></channel></rss>
